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And perhaps a longer solar cycle.


The sunspot cycle To comply with Wikipedia's this section of the article needs a complete rewrite.  maybe part of a longer activity period, says Richard Altrock, a U.S. Air Force scientist stationed at the National Solar Observatory The mission of the National Solar Observatory is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth, by providing forefront observational opportunities to the research community.  facility at Sacramento Peak, N.M. He adds that successive solar cycles may overlap.

Altrock bases his conclusions on 19 years of data gathered at the NSO NSO National Symphony Orchestra
NSO National Statistics Office (Philippines)
NSO National Solar Observatory
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. The studies indicate the full solar cycle may last nearly two decades. Moreover, the cylce may embrace other types of magnetic activity besides visible sunspots sunspots, dark, usually irregularly shaped spots on the sun's surface that are actually solar magnetic storms. The Chinese recorded dark features on the sun seen with the naked eye in 28 B.C. .

The sunspots cycle, determined by the number and position of the spots, typically has an 11-year period. Increased sunspot sunspot

Cooler-than-average region of gas on the Sun's surface associated with strong local magnetic activity. Sunspots appear as dark spots, but only in contrast with the surrounding photosphere, which is several thousand degrees hotter.
 formation at middle latitudes marks the beginning of each cycle. But other types of magnetic activity, which take place at higher latitudes - closer to the poles - precede sunspot formation, Altrock asserts.

Researchers had previously speculated that the solar activity cycle begins closer to the poles and then migrates to lower latitudes, Altrock notes. But high-latitude features on the surface of the sun are difficult to observe from Earth because the angle of sight distorts them or makes them invisible. To overcome this problem, Altrock and his colleagues restricted their observations to the corona, the region above the sun's visible surface. Since bright coronal cor·o·nal
adj.
1. Of or relating to a corona, especially of the head.

2. Of, relating to, or having the direction of the coronal suture or of the plane dividing the body into front and back portions.
 features correspond to magnetic activity on the surface, the researchers could deduce the location of magnetic features on the sun.

Using a coronagraph coronagraph (kərō`nəgrăf'), device invented by the French astronomer B. Lyot (1931) for the purpose of observing the corona of the sun and solar prominences occurring in the chromosphere.  to block the overwhelmingly bright light emitted by the solar surface, Altrock and his team measured faint emissions from the inner corona. Observations during the past 19 years by Altrock an others indicate that magnetic activity preceding the current sunspot cycle began at high solar latitudes in 1979. The full cycle is expected to last through 1998. The NSO studies also show that the next solar cycle, which should produce a peak number of sunspots just after the turnof the century, began in 1990 at a lattitude of 70 degrees, overlapping the current solar cycle. This cycle may also last about 19 years.
COPYRIGHT 1992 Science Service, Inc.
No portion of this article can be reproduced without the express written permission from the copyright holder.
Copyright 1992, Gale Group. All rights reserved. Gale Group is a Thomson Corporation Company.

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Article Details
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Title Annotation:sunspot cycle research
Author:Cowen, Ron
Publication:Science News
Article Type:Brief Article
Date:Jun 20, 1992
Words:325
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